The serendipitous discovery of a group or cluster of young galaxies at z similar or equal to 2.40 in deep Hubble Space Telescope WFPC2 images

被引:44
作者
Pascarelle, SM
Windhorst, RA
Driver, SP
Ostrander, EJ
Keel, WC
机构
[1] UNIV ALABAMA,DEPT PHYS & ASTRON,TUSCALOOSA,AL 35487
[2] AURA INC,SPACE TELESCOPE SCI INST,NASA ESA HUBBLE SPACE TELESCOPE,TUCSON,AZ
[3] UNIV ARIZONA,SMITHSONIAN INST,MULTIPLE MIRROR TELESCOPE OBSERV,TUCSON,AZ 85721
[4] UNIV ARIZONA,STEWARD OBSERV,TUCSON,AZ 85721
[5] CALTECH,CARNEGIE INST WASHINGTON,PALOMAR OBSERV,PASADENA,CA 91125
关键词
galaxies; clusters; general; distances and redshifts; evolution; formation; quasars;
D O I
10.1086/309852
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report the serendipitous discovery of a group or cluster of young galaxies at z similar or equal to 2.40 in a 24 orbit Hubble Space Telescope/WFPC2 exposure of the field around the weak radio galaxy 53W002. Potential cluster members were identified on ground-based narrowband redshifted Ly alpha images and confirmed via spectroscopy. In addition to the known weak radio galaxy 53W002 at z = 2.390, two other objects were found to have excess narrowband Lya! emission at z similar or equal to 2.40. Both have been spectroscopically confirmed, and one clearly contains a weak active galactic nucleus (AGN). They are located within 1' of 53W002 or similar to 0.23 h(100)(-1) Mpc (q(0) = 0.5) at z similar or equal to 2.40, which is the physical scale of a group or small cluster of galaxies. Profile fitting of the WFPC2 images shows that the objects are very compact, with scale lengths similar or equal to 0''.1 (similar or equal to 0.39 h(100)(-1) kpc), and are rather faint (luminosities < L*), implying that they may be subgalactic-sized objects. We discuss these results in the context of galaxy and cluster evolution and the role that weak AGNs may play in the formation of young galaxies.
引用
收藏
页码:L21 / &
页数:6
相关论文
共 32 条
[1]  
[Anonymous], APJ
[2]   SPECTRAL EVOLUTION OF GALAXIES .1. EARLY-TYPE SYSTEMS [J].
BRUZUAL, G .
ASTROPHYSICAL JOURNAL, 1983, 273 (01) :105-127
[3]  
CALZETTI D, 1992, APJ, V399, P39
[4]   STRUCTURAL PARAMETERS OF FAINT GALAXIES FROM PREREFURBISHMENT HUBBLE-SPACE-TELESCOPE MEDIUM DEEP SURVEY OBSERVATIONS [J].
CASERTANO, S ;
RATNATUNGA, KU ;
GRIFFITHS, RE ;
IM, M ;
NEUSCHAEFER, LW ;
OSTRANDER, EJ ;
WINDHORST, RA .
ASTROPHYSICAL JOURNAL, 1995, 453 (02) :599-610
[5]  
COWIE LL, 1989, APJ, V336, P41
[6]   DISCOVERY OF A PROBABLE GALAXY WITH A REDSHIFT OF 3.218 [J].
DJORGOVSKI, S ;
SPINRAD, H ;
MCCARTHY, P ;
STRAUSS, MA .
ASTROPHYSICAL JOURNAL, 1985, 299 (01) :L1-&
[7]   A CLUSTER OF NASCENT GALAXIES AT Z=2 [J].
DRESSLER, A ;
OEMLER, A ;
GUNN, JE ;
BUTCHER, H .
ASTROPHYSICAL JOURNAL, 1993, 404 (02) :L45-&
[8]   THE MORPHOLOGICAL MIX OF FIELD GALAXIES TO M(I)=24.25 MAGNITUDES (B(J)SIMILAR-TO-26 MAGNITUDES) FROM A DEEP HUBBLE-SPACE-TELESCOPE WFPC2 IMAGE [J].
DRIVER, SP ;
WINDHORST, RA ;
WINDHORST, A ;
OSTRANDER, EJ ;
KEEL, WC ;
GRIFFITHS, RE ;
RATNATUNGA, KU .
ASTROPHYSICAL JOURNAL, 1995, 449 (01) :L23-L27
[9]   EMISSION FROM THE Z = 2 DAMPED LY-ALPHA ABSORBER TOWARD Q1215+333 [J].
ELSTON, R ;
BECHTOLD, J ;
LOWENTHAL, J ;
RIEKE, M .
ASTROPHYSICAL JOURNAL, 1991, 373 (02) :L39-L42
[10]  
FRANCIS PJ, 1996, IN PRESS APJ